A Convolutional Neural Network for Multiple Particle Identification in the Microboone Liquid Argon Time Projection Chamber
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Decays of the Tau Lepton*
SLAC - 292 UC - 34D (E) DECAYS OF THE TAU LEPTON* Patricia R. Burchat Stanford Linear Accelerator Center Stanford University Stanford, California 94305 February 1986 Prepared for the Department of Energy under contract number DE-AC03-76SF00515 Printed in the United States of America. Available from the National Techni- cal Information Service, U.S. Department of Commerce, 5285 Port Royal Road, Springfield, Virginia 22161. Price: Printed Copy A07, Microfiche AOl. JC Ph.D. Dissertation. Abstract Previous measurements of the branching fractions of the tau lepton result in a discrepancy between the inclusive branching fraction and the sum of the exclusive branching fractions to final states containing one charged particle. The sum of the exclusive branching fractions is significantly smaller than the inclusive branching fraction. In this analysis, the branching fractions for all the major decay modes are measured simultaneously with the sum of the branching fractions constrained to be one. The branching fractions are measured using an unbiased sample of tau decays, with little background, selected from 207 pb-l of data accumulated with the Mark II detector at the PEP e+e- storage ring. The sample is selected using the decay products of one member of the r+~- pair produced in e+e- annihilation to identify the event and then including the opposite member of the pair in the sample. The sample is divided into subgroups according to charged and neutral particle multiplicity, and charged particle identification. The branching fractions are simultaneously measured using an unfold technique and a maximum likelihood fit. The results of this analysis indicate that the discrepancy found in previous experiments is possibly due to two sources. -
Book of Abstracts
12th International Neutrino Summer School 2019 Monday 05 August 2019 - Friday 16 August 2019 Fermi National Accelerator Laboratory Book of Abstracts Contents Intro to Group Exercises .................................... 1 Neutrinos and nuclear non-proliferation ........................... 1 INSS2019 welcome and introduction .............................. 1 Solar and Reactor Neutrino Experiments ........................... 1 Precise Measurement of Reactor Antineutrino Oscillation Parameters and Fuel-dependent Variation of Antineutrino Yield and Spectrum at RENO ................. 1 Using Convolutional Neural Networks to Reconstruct Dead Channels in MicroBooNE . 1 Origin and Nature of Neutrino Mass I ............................. 2 Introduction to Leptogenesis .................................. 2 Origin and Nature of Neutrino Mass II ............................ 2 Direct Neutrino Mass Measurements ............................. 2 Neutrinoless Double-beta Decay Experiments ........................ 2 Neutrino Beams and Fluxes .................................. 3 Lepton-Nucleus Cross Section Theory ............................. 3 Neutrino Cross Section Experiments ............................. 3 Origin and Nature of Neutrino Mass III ............................ 3 Particle Astrophysics with High-Energy Neutrinos ..................... 3 Neutrino Detection II ...................................... 3 Phenomenology of Atmospheric and Accelerator Neutrinos ................ 3 Tau neutrinos and upward-going air showers: stochastic versus continuous -
Design and Construction of the Microboone Detector
BNL-113631-2017-JA Design and Construction of the MicroBooBE Detector The MicroBooNE Collaboration Submitted to Journal of Instrumentation January 17, 2017 Physics Department Brookhaven National Laboratory U.S. Department of Energy USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25) Notice: This manuscript has been co-authored by employees of Brookhaven Science Associates, LLC under Contract No. DE-SC0012704 with the U.S. Department of Energy. The publisher by accepting the manuscript for publication acknowledges that the United States Government retains a non-exclusive, paid-up, irrevocable, world-wide license to publish or reproduce the published form of this manuscript, or allow others to do so, for United States Government purposes. DISCLAIMER This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency thereof, nor any of their employees, nor any of their contractors, subcontractors, or their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or any third party’s use or the results of such use of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise, does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States Government or any agency thereof or its contractors or subcontractors. The views and opinions of authors expressed herein do not necessarily state or reflect those of the United States Government or any agency thereof. -
The Hunt for Sub-Gev Dark Matter at Neutrino Facilities: a Survey of Past and Present Experiments
Prepared for submission to JHEP The hunt for sub-GeV dark matter at neutrino facilities: a survey of past and present experiments Luca Buonocore,a;b Claudia Frugiuele,c;d Patrick deNivervillee;f aDipartimento di Fisica, Università di Napoli Federico II and INFN, Sezione di Napoli, I-80126 Napoli, Italy bPhysik Institut, Universität Zürich, CH-8057 Zürich, Switzerland cCERN, Theoretical Physics Departments, Geneva, Switzerland dINFN, Sezione di Milano, Via Celoria 16, I-20133 Milano, Italy. eCenter for Theoretical Physics of the Universe, IBS, Daejeon 34126, Korea f T2, Los Alamos National Laboratory (LANL), Los Alamos, NM, USA E-mail: [email protected], [email protected], [email protected] Abstract: We survey the sensitivity of past and present neutrino experiments to MeV-GeV scale vector portal dark matter and find that these experiments possess novel sensitivity that has not yet fully explored. Taking αD = 0:1 and a dark photon to dark matter mass ratio of three, the combined recast of previous analyses of BEBC and a projection of NOνA’s sensitivity are found to rule out the scalar thermal target for dark matter masses between 10 MeV to 100 MeV with existing data, while CHARM-II and MINERνA place somewhat weaker limits. These limits can be dramatically improved by off-axis searches using the NuMI beamline and the MicroBooNE, MiniBooNE or ICARUS detectors, and can even begin to probe the Majorana thermal target. We conclude that past and present neutrino facilities can search for light dark matter concurrently with their neutrino program and reach a competitive sensitivity to proposed future experiments. -
Introduction to Subatomic- Particle Spectrometers∗
IIT-CAPP-15/2 Introduction to Subatomic- Particle Spectrometers∗ Daniel M. Kaplan Illinois Institute of Technology Chicago, IL 60616 Charles E. Lane Drexel University Philadelphia, PA 19104 Kenneth S. Nelsony University of Virginia Charlottesville, VA 22901 Abstract An introductory review, suitable for the beginning student of high-energy physics or professionals from other fields who may desire familiarity with subatomic-particle detection techniques. Subatomic-particle fundamentals and the basics of particle in- teractions with matter are summarized, after which we review particle detectors. We conclude with three examples that illustrate the variety of subatomic-particle spectrom- eters and exemplify the combined use of several detection techniques to characterize interaction events more-or-less completely. arXiv:physics/9805026v3 [physics.ins-det] 17 Jul 2015 ∗To appear in the Wiley Encyclopedia of Electrical and Electronics Engineering. yNow at Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723. 1 Contents 1 Introduction 5 2 Overview of Subatomic Particles 5 2.1 Leptons, Hadrons, Gauge and Higgs Bosons . 5 2.2 Neutrinos . 6 2.3 Quarks . 8 3 Overview of Particle Detection 9 3.1 Position Measurement: Hodoscopes and Telescopes . 9 3.2 Momentum and Energy Measurement . 9 3.2.1 Magnetic Spectrometry . 9 3.2.2 Calorimeters . 10 3.3 Particle Identification . 10 3.3.1 Calorimetric Electron (and Photon) Identification . 10 3.3.2 Muon Identification . 11 3.3.3 Time of Flight and Ionization . 11 3.3.4 Cherenkov Detectors . 11 3.3.5 Transition-Radiation Detectors . 12 3.4 Neutrino Detection . 12 3.4.1 Reactor Neutrinos . 12 3.4.2 Detection of High Energy Neutrinos . -
Search for Electron Neutrinos in Multiple Topologies with the Microboone Experiment
Search for Electron Neutrinos in Multiple Topologies with the MicroBooNE Experiment MICROBOONE-NOTE-1085-PUB The MicroBooNE Collaboration June 23, 2020 Abstract This note presents the status of the measurement of electron neutrinos from the Fermilab Booster Neutrino Beamline (BNB) with the MicroBooNE experiment. The analysis is aimed at investigating the nature of the low energy excess of electromagnetic activity observed by the MiniBooNE experiment. The νe event selection relies on topological and calorimetric information to characterise particles produced in these interactions, leveraging the Pandora multi-algorithm reconstruction framework as well as custom particle identification and pattern recognition tools. Results presented in this note use 5:88 × 1020 protons on target of data collected between 2015 and 2018. These include the performance of particle identification tools for µ/p and e/γ separation, along with electromagnetic shower calibration with the largest sample of π0 events measured on argon. Progress towards the completion of this analysis is shown through the measurement of high-energy charged-current νe interactions and their kinematic distributions using both inclusive (1eX) and exclusive (1e0p0π and 1eNp0π) channels. Measurements of charged-current νµ interactions aimed at constraining flux and cross-section systematic uncertainties are also shown. We present the analysis' preliminary sensitivity of an electron-like signal hypothesis to the MiniBooNE excess which includes flux, cross-section, and detector systematic uncertainties. 1 Contents 1 Introduction 3 2 Analysis Approach3 3 Event Reconstruction and Analysis Tools4 4 Electron Neutrino Event Selection7 5 Muon Neutrino Constraint, Systematics, and Analysis Sensitivity 13 6 Selected Electron Neutrinos at High Energy 15 7 Conclusions 16 A Measuring Electron Neutrinos with Particle Identification in the MicroBooNE LArTPC for sensitivity to new Physics 17 B Charged-Current Electron Neutrino Measurement with the MicroBooNE De- tector 20 B.1 Electron identification.................................. -
Machine-Learning-Based Global Particle-Identification Algorithms At
Machine-Learning-based global particle-identification algorithms at the LHCb experiment Denis Derkach1;2, Mikhail Hushchyn1;2;3, Tatiana Likhomanenko2;4, Alex Rogozhnikov2, Nikita Kazeev1;2, Victoria Chekalina1;2, Radoslav Neychev1;2, Stanislav Kirillov2, Fedor Ratnikov1;2 on behalf of the LHCb collaboration 1 National Research University | Higher School of Economics, Moscow, Russia 2 Yandex School of Data Analysis, Moscow, Russia 3 Moscow Institute of Physics and Technology, Moscow, Russia 4 National Research Center Kurchatov Institute, Moscow, Russia E-mail: [email protected] Abstract. One of the most important aspects of data analysis at the LHC experiments is the particle identification (PID). In LHCb, several different sub-detectors provide PID information: two Ring Imaging Cherenkov (RICH) detectors, the hadronic and electromagnetic calorimeters, and the muon chambers. To improve charged particle identification, we have developed models based on deep learning and gradient boosting. The new approaches, tested on simulated samples, provide higher identification performances than the current solution for all charged particle types. It is also desirable to achieve a flat dependency of efficiencies from spectator variables such as particle momentum, in order to reduce systematic uncertainties in the physics results. For this purpose, models that improve the flatness property for efficiencies have also been developed. This paper presents this new approach and its performance. 1. Introduction Particle identification (PID) algorithms play a crucial part in any high-energy physics analysis. A higher performance algorithm leads to a better background rejection and thus more precise results. In addition, an algorithm is required to work with approximately the same efficiency in the full available phase space to provide good discrimination for various analyses. -
Arxiv:1804.03238V1 [Hep-Ex] 9 Apr 2018
SNSN-323-63 April 11, 2018 Neutrino Cross Sections: Status and Prospects M. F. Carneiro1 Department of Physics, Oregon State University, Corvallis, Oregon 97331, USA We summarize the current status of accelerator based neutrino cross- section measurements. We focus on the experimental challenges while also presenting the motivation for these measurements. Selected results are highlighted after a quick description of the current major collaborations working on the field. PRESENTED AT arXiv:1804.03238v1 [hep-ex] 9 Apr 2018 NuPhys2017, Prospects in Neutrino Physics Barbican Centre, London, UK, December 20{22, 2017 1This work was supported by NSF Award PHY-1505472. 1 Introduction Neutrino physics is entering a new era of precision measurements and cross section measurements play a vital part. We will not discuss in details the effect of cross section measurements on systematic uncertainties as it has been well described in the literature [1, 2, 3, 4], but rather focus on the experimental difficulties of these measurements as well as show the shortcomings of the current theoretical models de- scribing neutrino-nucleus scattering. We also highlight new results from MINERvA, MicroBooNE, NoVA and T2K which have been released or presented in public con- ferences prior to the time of the NuPhys Workshop (December 2017) as well as given a quick description of each experiment. In Section 1, we discuss the common general goals of the program; in Section 2 we present the experimental difficulties involved in these measurements; Section 3 have a quick description of the effects for oscillation experiments; in Section 4 highlight new results and in Section 5 we summarize and discuss future directions. -
Luke Pickering on Behalf of NUISANCE
nuisance.hepforge.org github.com/NUISANCEMC/nuisance nuisance-xsec.slack.com [email protected] Luke Pickering on behalf of NUISANCE NuSTEC board meeting 2019 ● T2K, MINERvA, DUNE collaborators ● A breadth of experience using GENIE, NuWro, NEUT, GiBUU ● Have worked on neutrino cross-sections measurements, generators dev. and oscillation analyses on T2K and DUNE ● Stared at, thought about, and discussed a lot of neutrino interaction measurements (at NuSTEC and elsewhere) ● Developed interaction systematics for T2K and DUNE analyses ● Started as PhD project, now junior postdocs L. Pickering C. Wret C. Wilkinson ● What is NUISANCE? ● What have we done with NUISANCE? ● What do we plan to do with NUISANCE? ● How can NUISANCE be used in conjunction with NuSTEC? L. Pickering 3 ● Converts generator output from GENIE, NuWro, NEUT, GiBUU and NUANCE ● Uses a common event format with common functions (e.g. GetLepton(), GetQ2(), GetFinalState() ) With all generators in the same format, it’s easy to produce ● Generator-to-generator comparisons ● Model to model comparisons ● Comparison to data ● If event reweighting is available (GENIE, NEUT, NuWro): ○ Fit parameters to data ○ Evaluate uncertainty bands against data ○ Evaluate uncertainties against each other JINST 12 (2017) no. 01, P01016 L. Pickering 4 Compare effect of systematics on distributions from the same generator Effect of MAQE on generated NuWro events versus MiniBooNE CCQE data L. Pickering 5 Compare different generators and their models in a “flat-tree” format CC0π final state from NuWro with Nieves 2p2h CC0π final state from GENIE with Empirical 2p2h L. Pickering 6 Compare your favourite generators and models, which does best/worst? L. -
Particle Identification
Particle Identification Graduate Student Lecture Warwick Week Sajan Easo 28 March 2017 1 Outline Introduction • Main techniques for Particle Identification (PID) Cherenkov Detectors • Basic principles • Photodetectors • Example of large Cherenkov detector in HEP Detectors using Energy Loss (dE/dx) from ionization and atomic excitation Time of Flight (TOF) Detectors Transition Radiation Detectors (TRD) More Examples of PID systems • Astroparticle Physics . Not Covered : PID using Calorimeters . Focus on principles used in the detection methods. 2 Introduction . Particle Identification is a crucial part of several experiments in Particle Physics. • goal: identify long-lived particles which create signals in the detector : electrons, muons ,photons , protons, charged pions, charged kaons etc. • short-lived particles identified from their decays into long-lived particles • quarks, gluons : inferred from hadrons, jets of particles etc , that are created. In the experiments at the LHC: Tracking Detector : Directions of charged particles (from the hits they create in silicon detectors, wire chambers etc.) Tracking Detector + Magnet : Charges and momenta of the charged particles (Tracking system ) Electromagnetic Calorimeter (ECAL) : Energy of photons, electrons and positrons (from the energy deposited in the clusters of hits they create in the shape of showers ). Hadronic Calorimeter (HCAL) : Energy of hadrons : protons, charged pions etc. ( from the energy deposited in the clusters of hits they create in the shape of showers ) Muon Detector : Tracking detector for muons, after they have traversed the rest of the detectors 3 Introduction Some of the methods for particle identification: Electron : ECAL cluster has a charged track pointing to it and its energy from ECAL is close to its momentum from Tracking system. -
The ICARUS Experiment †
universe Communication The ICARUS Experiment † Christian Farnese and on behalf of the ICARUS Collaboration Dipartimento di Fisica ed Astronomia, Universita degli Studi di Padova, ed INFN, 35131 Sezione di Padova, Italy; [email protected] † This paper is based on the talk at the 7th International Conference on New Frontiers in Physics (ICNFP 2018), Crete, Greece, 4–12 July 2018. Received: 28 November 2018; Accepted: 25 January 2019; Published: 29 January 2019 Abstract: The 760-ton ICARUST600 detector has completed a successful three-year physics run at the underground LNGSlaboratories, searching for atmospheric neutrino interactions and, with the CNGSneutrino beam from CERN, performing a sensitive search for LSND-like anomalous ne appearance, which contributed to constraining the allowed parameters to a narrow region around Dm2 ∼ eV2, where all the experimental results can be coherently accommodated at 90% C.L. The T600 detector underwent a significant overhaul at CERN and has now been moved to Fermilab, to be soon exposed to the Booster Neutrino Beam (BNB) to search for sterile neutrinos within the SBNprogram, devoted to definitively clarifying the open questions of the presently-observed neutrino anomalies. This paper will address ICARUS’s achievements, its status, and plans for the new run and the ongoing analyses, which will be finalized for the next physics run at Fermilab. Keywords: neutrino physics; liquid argon; TPC 1. The ICARUS T600 Detector A very promising detection technique for the study of rare events such as the neutrino interactions is based on the Liquid Argon Time Projection Chamber (LAr-TPC). These detectors, first proposed by C.Rubbia in 1977 [1], combine the imaging capabilities of the famous bubble chambers with the excellent energy measurement of huge electronic detectors. -
Cosmic Ray Background Rejection with Wire-Cell Lartpc Event Reconstruction in Microboone
Cosmic Ray Background Rejection with Wire-Cell LArTPC Event Reconstruction in MicroBooNE MICROBOONE-NOTE-1084-PUB The MicroBooNE Collaboration∗ (Dated: June 20, 2020) For a large Liquid Argon Time Projection Chamber (LArTPC) operating on or near the surface to detect neutrino interactions, the rejection of cosmic background is a critical and challenging task because of the large cosmic ray flux and the slow timing of the TPC. In this paper, we introduce a superior cosmic background rejection procedure based on the Wire-Cell 3D event reconstruction for LArTPCs. The foundational reconstruction techniques including the 3D imaging and clustering of TPC ionization charge data, processing of PMT light data, and matching of the TPC charge and PMT light information are reviewed. This is followed by a detailed description of track trajectory fitting and dQ=dx determination. These reconstruction tools further enable various methods to tag cosmic-ray muons in time with the neutrino beam spills. From a hardware trigger level 1:20k neutrino to cosmic-ray background ratio, high-performance generic neutrino selection, i.e. cosmic- ray background rejection, is achieved in the MicroBooNE experiment with a cosmic contamination of 14.9% (9.7%) for the visible energy region greater than 0 (200) MeV. High efficiencies of neutrino interactions are also retained, and they are 80.4% and 87.6% for νµ charged-current and νe charged- current interactions, respectively. CONTENTS B. Stopped muon examples 23 I. Introduction 1 References 24 II. MicroBooNE detector and readout 3 I. INTRODUCTION III. Review of foundational reconstruction techniques 4 The liquid argon time projection chamber [1{4] A.